Sign on

SAO/NASA ADS Astronomy Abstract Service

· Find Similar Abstracts (with default settings below)
· Electronic Refereed Journal Article (HTML)
· Full Refereed Journal Article (PDF/Postscript)
· arXiv e-print (arXiv:astro-ph/0404549)
· References in the article
· Citations to the Article (234) (Citation History)
· Refereed Citations to the Article
· Also-Read Articles (Reads History)
· HEP/Spires Information
· Translate This Page
PSRCHIVE and PSRFITS: An Open Approach to Radio Pulsar Data Storage and Analysis
Hotan, A. W.; van Straten, W.; Manchester, R. N.
AA(Swinburne Centre for Astrophysics & Supercomputing, Hawthorn VIC 3122, Australia, Australia Telescope National Facility, Epping NSW 1710, Australia ), AB(Netherlands Foundation for Research in Astronomy, 7990 AA Dwingeloo, The Netherlands), AC(Australia Telescope National Facility, Epping NSW 1710, Australia)
Publications of the Astronomical Society of Australia, Volume 21, Issue 3, pp. 302-309. (PASA Homepage)
Publication Date:
Astronomy Keywords:
pulsars: general, methods: data analysis
Bibliographic Code:


A new set of software applications and libraries for use in the archival and analysis of pulsar astronomical data is introduced. Known collectively as the PSRCHIVE scheme, the code was developed in parallel with a new data storage format called PSRFITS, which is based on the Flexible Image Transport System (FITS). Both of these projects utilise a modular, object-oriented design philosophy. PSRCHIVE is an open source development environment that incorporates an extensive range of C++ object classes and pre-built command line and graphical utilities. These deal transparently and simultaneously with multiple data storage formats, thereby enhancing data portability and facilitating the adoption of the PSRFITS file format. Here, data are stored in a series of modular header-data units that provide flexibility and scope for future expansion. As it is based on FITS, various standard libraries and applications may be used for data input, output, and visualisation. Both PSRCHIVE and PSRFITS are made publicly available to the academic community in the hope that this will promote their widespread use and acceptance.
Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)


Find Similar Abstracts:

Use: Authors
Keywords (in text query field)
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
arXiv e-prints